Results 11 to 20 of about 26,451 (248)

Simulating Reionization: Character and Observability [PDF]

open access: yesAIP Conference Proceedings, 2007
In recent years there has been considerable progress in our understanding of the nature and properties of the reionization process. In particular, the numerical simulations of this epoch have made a qualitative leap forward, reaching sufficiently large ...
Bond, J. Richard   +5 more
core   +3 more sources

Cosmic Reionization in the JWST Era: Back to AGNs? [PDF]

open access: goldThe Astrophysical Journal
Deep surveys with the James Webb Space Telescope (JWST) have revealed an emergent population of moderate-luminosity, broad-line active galactic nuclei (AGNs) at 4 ≲ z ≲ 13 powered by accretion onto early massive black holes.
Piero Madau   +3 more
doaj   +2 more sources

The First Galaxies and the Likely Discovery of Their Fossils in the Local Group [PDF]

open access: yesAdvances in Astronomy, 2010
The lower bound for the mass of a galaxy is unknown, as are the typical luminosity of the smallest galaxies and their numbers. The answers depend on the extent to which star formation in the first population of small mass halos may be suppressed by ...
Massimo Ricotti
doaj   +4 more sources

Modeling cosmic reionization

open access: yesLiving Reviews in Computational Astrophysics, 2022
AbstractThe transformation of cold neutral intergalactic hydrogen into a highly ionized warm plasma marks the end of the cosmic dark ages and the beginning of the age of galaxies. The details of this process reflect the nature of the early sources of radiation and heat, the statistical characteristics of the large-scale structure of the Universe, the ...
Nickolay Y. Gnedin, Piero Madau
openaire   +2 more sources

CEMPlifying reionization [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
The massive stars that ionised the Universe have short lifetimes and can only be studied near the time of formation, but any low mass stars that formed contemporaneously might be observable in the local Universe today. We study the abundance pattern and spatial distribution of these `siblings of reionizers' (SoRs) in the EAGLE cosmological ...
Mahavir Sharma, Tom Theuns, Carlos Frenk
openaire   +3 more sources

The Impact of Patchy Reionization on Ultrafaint Dwarf Galaxies

open access: yesThe Astrophysical Journal, 2023
We investigate how patchy reionization affects the star formation history (SFH) and stellar metallicity of ultrafaint dwarf galaxies (UFDs). Patchy reionization refers to varying ultraviolet background strengths depending on a galaxy’s environment ...
Jaeeun Kim   +5 more
doaj   +1 more source

The Epoch of Reionization in Warm Dark Matter Scenarios

open access: yesUniverse, 2021
In this paper we investigate how the Reionization process is affected by early galaxy formation in different cosmological scenarios. We use a semi-analytic model with suppressed initial power spectra to obtain the UV Luminosity Function in thermal Warm ...
Massimiliano Romanello   +2 more
doaj   +1 more source

The epoch of reionization [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2006
We have modelled the process of reionization of the IGM by photoionization by galaxies, in order to predict the epoch of reionization. We use a sophisticated semi-analytic model to track the formation of galaxies. Our study represents a much more complete and physically consistent modelling of reionization than has been conducted in the past ...
Benson, A.J.   +3 more
openaire   +3 more sources

Dust distribution during reionization [PDF]

open access: yesAstronomy & Astrophysics, 2007
The dust produced by the first generation of stars will be a foreground to cosmic microwave background. In order to evaluate the effect of this early dust, we calculate the power spectrum of the dust emission anisotropies and compare it with the sensitivity limit of the Planck satellite.
Elfgren, E.   +2 more
openaire   +4 more sources

The reionization of carbon [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
Observations suggest that CII was more abundant than CIV in the intergalactic medium towards the end of the hydrogen reionization epoch. This transition provides a unique opportunity to study the enrichment history of intergalactic gas and the growth of the ionizing background (UVB) at early times.
Finlator, Kristian   +5 more
openaire   +3 more sources

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